First retrieval of fire radiative power from COMS data using the mid-infrared radiance method

Kim, Daesun; Cho, Jaeil; Hong, Sungwook; Lee, Hanlim; Won, Myoung-Soo; Byun, Sangwoo; Park, Kyungwon; Lee, Yang-Won

doi:10.1080/2150704x.2016.1239283

Cited by 4 publications

(1 citation statement)

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“…The mid-infrared region in the wavelength range of 3.5 to 4.1 µm features a high transmittance [1], and the gases that have an impact on the optical properties are water vapor, carbon dioxide, and methane [2]. In the spectral range of 3.60~3.85 µm, the influence of aerosol particles on the optical properties of the atmospheric window is much lower than that on those of the shortwave infrared atmospheric window [3][4][5]; especially under clean atmospheric conditions, the attenuation of total radiation mainly comes from water vapor and the contribution of aerosol particles to the total radiation attenuation is generally less than 5%, indicating good atmospheric penetration characteristics [6,7]. As a result, the mid-infrared band exhibits unique properties over the full wavelength range, unlike the VNIR and LWIR bands [8][9][10], allowing this channel to be suitable as a reference for calibration and verification.…”

Section: Introductionmentioning

confidence: 99%

Retrieval of an On-Orbit Bidirectional Reflectivity Reference in the Mid-Infrared Bands of FY-3D/MERSI-2 Channels 20

Peng,

Chen,

Wang

et al. 2023

Remote Sensing

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The acquisition of high-accuracy reflectance in mid-infrared channels is of great significance for the on-orbit cross-calibration of other bands using the mid-infrared band. However, due to the phenomenon that some sensors have a wide range of wavelengths covered by adjacent channels in the mid-infrared band, the traditional method of estimating the mid-infrared reflectivity assumes that the sea surface reflectivity in different mid-infrared bands is equal, which will lead to a large error during calculation. To solve this problem, this study proposes a nonlinear split-window algorithm involving ocean sun glint data to retrieve reflectivity of FY-3D/MERSI-2 channels 20. The results show that the variation range of sea surface reflectivity of channel 20 in the glint area is 10~25%, the mean value of the reflectivity difference obtained by the nonlinear split-window algorithm is 0.27%, and the RMSE is 0.0066. Among the main influencing factors, the atmospheric conditions have the greatest impact, and the effects of the uncertainties in the water vapor content and aerosol optical thickness on the calculation results are 1.16% and 0.34%, respectively. The initial value limits of the mid-infrared sea surface reflectivity also contribute approximately 0.84%, and their contribution to the uncertainty represents one of the main components. This work shows that the nonlinear split-window algorithm can calculate the infrared sea surface reflectivity with high accuracy and can be used as a reference for in-orbit cross-calibration between different bands.

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